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PHYS2021LYLE12168 PHYS

pH-based Cancer Detection by Graphene Quantum Dots

Type: Undergraduate
Author(s): Veronica Lyle Physics & Astronomy Matt Dadet Physics & Astronomy Bong Lee Physics & Astronomy
Advisor(s): Anton Naumov Physics & Astronomy Giridhar Akkaraju Biology Kat Barger Physics & Astronomy
Location: Zoom Room 5, 03:35 PM

Many cancers are characterized by rapid cell growth and division. This growth causes the area to become densely packed, forming tumors and therefore limiting oxygen penetration, and also causing the cell to have elevated energy needs. These factors trigger the use of mechanisms which have a high acidic output, which makes cancerous environments measurably more acidic than their healthy counterparts. This study was conducted to determine the suitability of various nanomaterial-based platforms for pH sensing as an additive to their previously shown suitability for drug/gene delivery and bioimaging. Several platforms were chosen, including Glucose-Doped Graphene Quantum Dots (GGQDs), Reduced Graphene Oxide-Derived Graphene Quantum Dots (RGQDs), and Aluminum-Doped Reduced Graphene Oxide-Derived Graphene Quantum Dots (Al-RGQDs), which all have peaks in their emission spectra in both the visible and infrared range. 9 spectra were taken from each of these platforms in the visible and infrared ranges from pH 6.00 to 8.00, as would be expected in cancerous and healthy biological systems. These spectra were then analyzed for defining characteristics which would distinguish between the various pH levels. While the results from GGQDs and RGQDs are thus far inconclusive, the relative peak intensity readings from the visible and infrared Al-RGQDs showed a promising inverse relationship that bears further investigation.

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PHYS2021MCKINNEY45065 PHYS

Hydrogenation of Reduced Graphene Oxide via Water Electrolysis

Type: Undergraduate
Author(s): Ryan McKinney Physics & Astronomy Debora Beeri Chemistry & Biochemistry Anton Naumov Physics & Astronomy Benjamin Sherman Chemistry & Biochemistry
Advisor(s): Anton Naumov Physics & Astronomy
Location: Zoom Room 5, 01:02 PM

Hydrogen energy is the most sustainable source of energy known to man. Though Earth has a seemingly limitless supply of hydrogen trapped in water molecules, industrial size production and storage of it has remained costly and dangerous. Reduced graphene oxide (rGO) shows great potential as a storage vessel for hydrogen while acting as a “catchers’ glove” for hydrogen when it is split from water. Where others have tried to store hydrogen in rGO by having it surrounded by hydrogen gas, I will attempt to directly attract hydrogen to rGO by taking advantage of hydrogen’s electrical attraction to rGO once it is split from water via electrolysis. This technique, paired with a novel method of preparation of the working cathode , could increase hydrogen storage in rGO that has not been achieved; furthering its potential as a safe, cost effective, and reversible hydrogen storage vessel.

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PHYS2021RIDDLE65157 PHYS

Forensic Astronomy: Collecting Chemical Fingerprints of Ancient Supernova Explosions

Type: Undergraduate
Author(s): Nicole Riddle Physics & Astronomy Emilie Burnham Physics & Astronomy
Advisor(s): Peter Frinchaboy Physics & Astronomy
Location: Zoom Room 2, 03:11 PM

The creation and evolution of elements, as a function of age, throughout the Milky Way disk provides a key constraint for galaxy evolution models. In an effort to provide these constraints, we have conducted an investigation into the rapid and slow-process neutron capture elemental abundances, which are created in supernovae, for a large sample of open clusters. Stars were identified as cluster members by the Open Cluster Chemical Abundance & Mapping (OCCAM) survey, which culls member candidates by Doppler velocity, metallicity, and proper motion from the observed OCCAM sample. We’ve obtained new data for neutron-capture elements in these clusters using the Subaru Observatory 8-m telescope in Hawaii with the High Dispersion Spectrograph (HDS). We are analyzing the neutron capture abundances in star clusters to measure the chemical evolution of the Milky Way.

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PHYS2021VASIREDDY13499 PHYS

Near-Infrared Fluorescence Imaging in Mice with Graphene Quantum Dots

Type: Undergraduate
Author(s): Satvik Vasireddy Physics & Astronomy Md. Tanvir Hasan Physics & Astronomy
Advisor(s): Anton Naumov Physics & Astronomy
Location: Zoom Room 4, 12:54 PM

In recent times, nanomaterials have attracted interest in the scientific community due to their capacity for drug/gene delivery as well as their ability to target tissues and serve as probes for delivery pathways through various bioimaging approaches. Nanomaterial-based imaging systems in the near-infrared (NIR) region are desirable in vivo due to low biological autofluorescence, low tissue scattering, and increased penetration depth in animal tissue. However, low biocompatibility, as well as complexity in preparation, impede many current NIR imaging platforms from biomedical applications. In order to rectify this issue, we developed biocompatible NIR emitting graphene quantum dots (GQDs) and tested them for imaging in animal tissues. GQDs injected into mice intravenously through the tail vein show NIR emission in multiple organs including the intestine, kidney, spleen, and liver. Localization of both quantum dots in these organs was verified through the NIR fluorescence microscopy of organ slices, taken at multiple time points (1, 3, 6, 24 hours) via hyperspectral fluorescence microscopy. Slices in the 6 hour time point show the strongest fluorescence and characteristic GQD spectral signatures at ~950 nm compared to none in the control slices. These results indicate that GQDs show promising potential for future applications in theranostics, for instance as imaging or image-guided drug delivery agents.

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PHYS2021WILSON33068 PHYS

New Tricks with the Joker: Revealing Binary Stars

Type: Undergraduate
Author(s): Mikayla Wilson Physics & Astronomy Nicole Riddle Physics & Astronomy
Advisor(s): Peter Frinchaboy Physics & Astronomy
Location: Zoom Room 5, 01:50 PM

Fifty percent of stars in the night sky are actually binary star systems, but finding and characterizing them require significant data, time, and analysis. Studying the brighter star of the pair is fairly straightforward, but the secondary is commonly hidden. Using the infrared spectroscopy data from the Sloan Digital Sky Survey combined with The Joker, a new Monte Carlo analysis technique, we are working to reveal and characterize these hidden binary stars.

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